First detection of ultra-fast outflows in a quiescent galaxy

Outflows in active galactic nuclei (AGN) are recognized as a fundamental mechanism driving the co-evolution of supermassive black holes (SMBHs) and their host galaxies. Although powerful outflows are frequently detected in gas-rich, active star-forming galaxies, their existence and potential impact within gas-poor, quiescent galaxies remain poorly understood. We report the first detection of a powerful ultra-fast outflow (UFO) in a nearby quiescent galaxy KUG 1208+386, providing a multiscale analysis of AGN winds from nuclear to galactic scales. We detect a nuclear X-ray UFO with a velocity of v out about-0.07c and a kinetic power of UFO=(0.8--6.5) times 10 43 erg/s, sufficient to drive effective AGN feedback (UFO/L Edd=(1--8)%) and far exceeding the galactic [OIII] outflow power about 10 40 erg/s. Host galaxy analysis reveals a massive quiescent system (specific star formation rate about3 times10-12 yr-1) that has been quenched about 9 Gyr ago. The central AGN is obscured by a line-of-sight (LOS) column density of (N H LOS/cm-2) about23 and the circumnuclear scattering material is Compton-thick (N H scatter/cm-2)=24.7+0.8-0.5. The discovery of a nuclear UFO in a long-quenched massive galaxy challenges the paradigm that UFOs are exclusive to gas-rich, star-forming systems, suggesting instead that they are governed by the local circumnuclear environments, rather than the global gas reservoir. Our results indicate that episodic, powerful winds can maintain the quiescent state of KUG 1208+386 over Gyr timescales, supporting a wind-driven `maintenance' mode of AGN feedback that is distinct from the classical jet mode.